High-significance Sunyaev-Zel'dovich measurement: Abell 1914 seen with the Arcminute Microkelvin Imager
arXiv:astro-ph/0509215 · doi:10.1111/j.1745-3933.2006.00151.x
Abstract
We report the first detection of a Sunyaev-Zel'dovich (S-Z) decrement with the Arcminute Microkelvin Imager (AMI). We have made commissioning observations towards the cluster A1914 and have measured an integrated flux density of -8.61 mJy in a uv-tapered map with noise level 0.19 mJy/beam. We find that the spectrum of the decrement, measured in the six channels between 13.5-18GHz, is consistent with that expected for a S-Z effect. The sensitivity of the telescope is consistent with the figures used in our simulations of cluster surveys with AMI.
arXiv comment5 pages, 6 figures, submitted to MNRAS Letters
References in corpus (19)
- Cosmology with the Sunyaev-Zel'dovich Effect
- The Sunyaev-Zel'dovich Effect
- The ROSAT Brightest Cluster Sample (BCS) - I. The compilation of the sample and the cluster log N-log S distribution
- The Northern ROSAT All-Sky (NORAS) Galaxy Cluster Survey I: X-ray Properties of Clusters Detected as Extended X-ray Sources
- Relativistic corrections to the Sunyaev-Zel'dovich effect
- A New Measurement of the X-ray Temperature Function of Clusters of Galaxies
- Galaxy Cluster Gas Mass Fractions from Sunyaev-Zel'dovich Effect Measurements: Constraints on Omega_M
- Measurements of the Sunyaev-Zeldovich Effect in the Nearby Clusters A478, A2142 and A2256
- The Atacama Cosmology Telescope
- 9C: A Survey of Radio Sources at 15 GHz with the Ryle Telescope
- Expectations For an Interferometric Sunyaev-Zel'dovich Effect Survey for Galaxy Clusters
- Limits on the Peculiar Velocities of Two Distant Clusters Using the Kinematic Sunyaev-Zel'dovich Effect
- Surveying the Sky with the Arcminute MicroKelvin Imager: Expected Constraints on Galaxy Cluster Evolution and Cosmology
- Submillimeter detection of the Sunyaev -- Zel'dovich effect toward the most luminous X-ray cluster at z=0.45
- H0 from an orientation-unbiased sample of SZ and X-ray clusters
- Determining the Hubble Constant from Ryle Telescope observations
- Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters
- An Unbiased Measurement of Ho through Cosmic Background Imager Observations of the Sunyaev-Zel'dovich Effect in Nearby Galaxy Clusters
- Studying Dark Energy with Galaxy Cluster Surveys
Cited by in corpus (12)
- The Arcminute Microkelvin Imager
- Exact reconstruction with directional wavelets on the sphere
- A Lensing Survey of X-ray Luminous Galaxy Clusters at Redshift z ~ 0.2: II: CFH12k Weak Lensing Analysis and Global Correlations
- The CMB temperature bispectrum induced by cosmic strings
- Bayesian modelling of clusters of galaxies from multi-frequency pointed Sunyaev--Zel'dovich observations
- The Sunyaev-Zel'dovich Effect at Five Arc-seconds: RXJ1347.5-1145 Imaged by ALMA
- Compressed sensing reconstruction of a string signal from interferometric observations of the cosmic microwave background
- All sky CMB map from cosmic strings integrated Sachs-Wolfe effect
- Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases
- Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters
- Wavelet domain Bayesian denoising of string signal in the cosmic microwave background
- Imaging Simulations of the Sunyaev-Zel'dovich Effect for ALMA